elib
DLR-Header
DLR-Logo -> http://www.dlr.de
DLR Portal Home | Imprint | Privacy Policy | Contact | Deutsch
Fontsize: [-] Text [+]

Three-dimensional spatial structures of solar wind turbulence from 10 000-km to 100-km scales

Narita, Y. and Glassmeier, K.H. and Goldstein, M.L. and Motschmann, U. and Sahraoui, F. (2011) Three-dimensional spatial structures of solar wind turbulence from 10 000-km to 100-km scales. Annales Geophysicae, 29, pp. 1731-1738. Copernicus Publications. DOI: 10.5194/angeo-29-1731-2011

[img]
Preview
PDF
522kB

Abstract

Using the four Cluster spacecraft, we have determined the three-dimensional wave-vector spectra of fluctuating magnetic fields in the solar wind. Three different solar wind intervals of Cluster data are investigated for this purpose, representing three different spatial scales: 10 000 km, 1000 km, and 100 km. The spectra are determined using the wave telescope technique (k-filtering technique) without assuming the validity of Taylor�s frozen-in-flow hypothesis nor are any assumptions made as to the symmetry properties of the fluctuations. We find that the spectra are anisotropic on all the three scales and the power is extended primarily in the directions perpendicular to the mean magnetic field, as might be expected of two-dimensional turbulence, however, the analyzed fluctuations are not axisymmetric. The lack of axisymmetry invalidates some earlier techniques using single spacecraft observations that were used to estimate the percentage of magnetic energy residing in quasitwo- dimensional power. However, the dominance of twodimensional turbulence is consistent with the relatively long mean free paths of cosmic rays in observed in the heliosphere. On the other hand, the spectra also exhibit secondary extended structures oblique from the mean magnetic field direction. We discuss possible origins of anisotropy and asymmetry of solar wind turbulence spectra.

Item URL in elib:https://elib.dlr.de/73308/
Document Type:Article
Title:Three-dimensional spatial structures of solar wind turbulence from 10 000-km to 100-km scales
Authors:
AuthorsInstitution or Email of AuthorsAuthors ORCID iD
Narita, Y.Institut für Geophysik und Meteorologie, TU Braunschweig, GermanyUNSPECIFIED
Glassmeier, K.H.Institut für Geophysik und Meteorologie, TU Braunschweig, GermanyUNSPECIFIED
Goldstein, M.L.Geospace Physics Laboratory, Code 673, Goddard Space Flight Center, Greenbelt, MD 20771, USAUNSPECIFIED
Motschmann, U.uwe.motschmann (at) dlr.deUNSPECIFIED
Sahraoui, F.Laboratoire de Physique des Plasmas Observatoire de Saint-Maur, 4 avenue de Neptune, 94107 Saint-Maur-Des-Foss´es,UNSPECIFIED
Date:2011
Journal or Publication Title:Annales Geophysicae
Refereed publication:Yes
Open Access:Yes
Gold Open Access:Yes
In SCOPUS:Yes
In ISI Web of Science:Yes
Volume:29
DOI :10.5194/angeo-29-1731-2011
Page Range:pp. 1731-1738
Publisher:Copernicus Publications
Status:Published
Keywords:Interplanetary physics (Interplanetary magnetic fields; MHD waves and turbulence; Plasma waves and turbulence)
HGF - Research field:Aeronautics, Space and Transport (old)
HGF - Program:Space (old)
HGF - Program Themes:W EW - Erforschung des Weltraums
DLR - Research area:Space
DLR - Program:W EW - Erforschung des Weltraums
DLR - Research theme (Project):W - Vorhaben Planetenforschung (old)
Location: Berlin-Adlershof
Institutes and Institutions:Institute of Planetary Research > Asteroids and Comets
Deposited By: Pieth, Susanne
Deposited On:10 Jan 2012 10:02
Last Modified:08 Mar 2018 18:47

Repository Staff Only: item control page

Browse
Search
Help & Contact
Information
electronic library is running on EPrints 3.3.12
Copyright © 2008-2017 German Aerospace Center (DLR). All rights reserved.